EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment GI001B_2. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Mon Dec 13 22:12:57 CET 2004 brunthaler@jive.nl

General Comments. ( Brief data summary and scan listing )
This is an Global experiment at 18cm, recorded at 256 Mbps on 07 June 2004. There are 2 polarisations and 4 subbands. Three subbands have 32 channels, while one subband has 512 channels in L and R polarisations. The experiment was correlated in three passes, where the pass one contained the 3 continuum IFs, pass 2 contains the spectral line LL-pol data and pass 3 contains the spectral line RR-pol data. Participating stations were EF, WB, MC, NT, TR, HH, JB and all VLBA stations.

The EVN reliability indicator (ERI) for this experiment was ERI=ERI*=0.95 (Ef=1, Wb=1, Mc=1, Nt=1, Tr=1, Hh=1, Jb=0.83).

Plots of the autocorrelations .
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Plots of the uncalibrated amplitude and phase against time .
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Plots of the uncalibrated amplitude and phase against frequency channel .
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The uncalibrated amplitude and phase of the crosshand correlations against frequency channel (not available) .
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TSYS against time .
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Telescope sensitivities from the a priori TSYS and Gain curves (the square of this number gives the antenna noise (SEFD) in Jy - the smaller the better).
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Fringe-fit phase solutions (including Parallactic Angle correction).
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Fringe-fit delay solutions .
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Fringe-fit rate solutions .
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Telescope bandpasses .
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Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
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Calibrated amplitude and phase against frequency channel .
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Naturally weighted dirty map produced before self-cal of:
1830+139: postscript , or FITS .
2145+067: postscript , or FITS .
OT081: postscript , or FITS .
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Uniformly weighted dirty map produced before self-cal of:
1830+139: postscript , or FITS .
2145+067: postscript , or FITS .
OT081: postscript , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
1830+139.
2145+067.
OT081.
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
1830+139: postscript , or text file .
2145+067: postscript , or text file .
OT081: postscript , or text file .
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Telescope sensitivities (the total AMP gain applied during both a priori and self calibration; the square of this number gives the antenna noise (SEFD) in Jy).
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Residual closure phase (visibility closure phase with model closure phase subtracted) for:
1830+139 .
2145+067 .
OT081 .
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Calibrated visibilities and the source model of:
1830+139 .
2145+067 .
OT081 .
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Calibrated visibilities against u,v distance for:
1830+139. postscript , or png (smaller)
2145+067. postscript , or png (smaller)
OT081. postscript , or png (smaller)
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u,v coverage for:
1830+139. postscript , or png (smaller)
2145+067. postscript , or png (smaller)
OT081. postscript , or png (smaller)
Comments.

1830+139: postscript , or FITS .
2145+067: postscript , or FITS .
OT081: postscript , or FITS .
Comments.